Ultraluminous X-ray sources

P Kaaret, H Feng, TP Roberts - Annual Review of Astronomy …, 2017 - annualreviews.org
We review observations of ultraluminous X-ray sources (ULXs). X-ray spectroscopic and
timing studies of ULXs suggest a new accretion state distinct from those seen in Galactic …

A CEERS discovery of an accreting supermassive black hole 570 Myr after the Big Bang: identifying a progenitor of massive z> 6 quasars

RL Larson, SL Finkelstein, DD Kocevski… - The Astrophysical …, 2023 - iopscience.iop.org
We report the discovery of an accreting supermassive black hole at z= 8.679. This galaxy,
denoted here as CEERS_1019, was previously discovered as a Lyα-break galaxy by …

Formation of the first stars and black holes

L Haemmerlé, L Mayer, RS Klessen, T Hosokawa… - Space Science …, 2020 - Springer
We review the current status of knowledge concerning the early phases of star formation
during cosmic dawn. This includes the first generations of stars forming in the lowest mass …

Radiation backgrounds at cosmic dawn: X-rays from compact binaries

P Madau, T Fragos - The Astrophysical Journal, 2017 - iopscience.iop.org
We compute the expected X-ray diffuse background and radiative feedback on the
intergalactic medium (IGM) from X-ray binaries prior to and during the epoch of reionization …

Building up the Population III initial mass function from cosmological initial conditions

A Stacy, V Bromm, AT Lee - Monthly Notices of the Royal …, 2016 - academic.oup.com
We simulate the growth of a Population III stellar system, starting from cosmological initial
conditions at z= 100. We follow the formation of a minihalo and the subsequent collapse of …

Galaxy properties and UV escape fractions during the epoch of reionization: results from the renaissance simulations

H Xu, JH Wise, ML Norman, K Ahn… - The Astrophysical …, 2016 - iopscience.iop.org
Cosmic reionization is thought to be primarily fueled by the first generations of galaxies. We
examine their stellar and gaseous properties, focusing on the star formation rates and the …

Impact of the cosmic background radiation on the initial mass function of metal-poor stars

S Chon, H Ono, K Omukai… - Monthly Notices of the …, 2022 - academic.oup.com
We study star cluster formation at low metallicities of Z/Z⊙= 10− 4–10− 1 using three-
dimensional hydrodynamics simulations. Particular emphasis is put on how the stellar mass …

The birth of a massive first-star binary

K Sugimura, T Matsumoto, T Hosokawa… - The Astrophysical …, 2020 - iopscience.iop.org
We study the formation of massive Population III binary stars using a newly developed
radiation hydrodynamics code with the adaptive mesh refinement and adaptive ray-tracing …

thesan-hr: galaxies in the Epoch of Reionization in warm dark matter, fuzzy dark matter, and interacting dark matter

X Shen, J Borrow, M Vogelsberger… - Monthly Notices of …, 2024 - academic.oup.com
Using high-resolution cosmological radiation-hydrodynamic (RHD) simulations (thesan-hr),
we explore the impact of alternative dark matter (altDM) models on galaxies during the …

Trap** of H ii regions in Population III star formation

O Jaura, SCO Glover, KMJ Wollenberg… - Monthly Notices of …, 2022 - academic.oup.com
Radiative feedback from massive Population III (Pop III) stars in the form of ionizing and
photodissociating photons is widely believed to play a central role in shutting off accretion …